Testing the X-ray reverberation model KYNREFREV in a sample of Seyfert 1 Active Galactic Nuclei

Understand

We present the first results obtained by the application of the KYNREFREV-reverberation model, which is ready for its use in XSPEC.

• This model computes the time dependent reflection spectra of the disc as a response to a flash of primary power-law radiation from a point source corona located on the axis of the black hole accretion disc (lamp-post geometry).
• Full relativistic effects are taken into account.
• The ionisation of the disc is set for each radius according to the amount of the incident primary flux and the density of the accretion disc.